Halo Formation from Yukawa Forces in the Very Early Universe
arXiv:2304.13053 · doi:10.1103/PhysRevD.108.103543
Abstract
If long-range attractive forces exist and are stronger than gravity then cosmic halo formation can begin in the radiation-dominated era. We study a simple realization of this effect in a system where dark matter fermions have Yukawa interactions mediated by scalar particles, analogous to the Higgs boson in the standard model. We develop a self-consistent description of the system including exact background dynamics of the scalar field, and precise modelling of the fermion density fluctuations. For the latter, we provide accurate approximations for the linear growth as well as quantitative modelling of the nonlinear evolution using N-body simulations. We find that halo formation occurs exponentially fast and on scales substantially larger than simple estimates predict. The final fate of these halos remains uncertain, but could be annihilation, dark stars, primordial black holes, or even the existence of galaxy-sized halos at matter-radiation equality. More generally, our results demonstrate the importance of mapping scalar-mediated interactions onto structure formation outcomes and constraints for beyond the standard model theories.
22 pages + references, 13 figures. Matches published version
References in corpus (22)
- Array Programming with NumPy
- Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC
- Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
- Cosmology and the Fate of Dilatation Symmetry
- Primordial Black Holes as Dark Matter: Recent Developments
- Stress Testing CDM with High-redshift Galaxy Candidates
- Growing Matter
- Large-scale dark matter simulations
- Growing neutrinos and cosmological selection
- Extreme Value Statistics of the Halo and Stellar Mass Distributions at High Redshift: are JWST Results in Tension with ΛCDM?
- Primordial seeds of supermassive black holes
- Constraining the primordial black hole scenario with Bayesian inference and machine learning: the GWTC-2 gravitational wave catalog
- Clarifying spherical collapse in coupled dark energy cosmologies
- Unveiling dark fifth forces with linear cosmology
- Spherical Collapse and Cluster Counts in Modified Gravity Models
- Small-scale shear: Peeling off diffuse subhalos with gravitational waves
- Dynamics of neutrino lumps in growing neutrino quintessence
- Primordial black holes as a dark matter candidate in theories with supersymmetry and inflation
- Cosmology of strongly interacting fermions in the early universe
- Condensed dark matter with a Yukawa interaction
- Particle linear theory on a self-gravitating perturbed cubic Bravais lattice
- Gravitational waves from rapid structure formation on microscopic scales before matter-radiation equality
Cited by in corpus (15)
- Primordial Black Holes from Supercooled Phase Transitions
- A double take on early and interacting dark energy from JWST
- Probing modified Hawking evaporation with gravitational waves from the primordial black hole dominated universe
- Compact objects in and beyond the Standard Model from non-perturbative vacuum scalarization
- Feeding plankton to whales: high-redshift supermassive black holes from tiny black hole explosions
- Primordial black holes as cosmic expansion accelerators
- Black Holes from Fermi Ball Collapse
- Late-forming black holes and the antiproton, gamma-ray, and anti-helium excesses
- Q-Balls in the presence of attractive force
- Observational Constraints on Early Coupled Quintessence
- Probing Long-Range Forces Between Neutrinos with Cosmic Structures
- Primordial black hole driven cosmic acceleration
- Inflation with the Trace Anomaly Action and Primordial Black Holes
- Dimming Starlight with Dark Compact Objects
- The Dark Side of the Moon: Listening to Scalar-Induced Gravitational Waves